Http://chandra.h arvard.edu/phot o/2007/m51/. Confronting Stellar Feedback Simulations with Observations of Hot Gas in Elliptical Galaxies Q. Daniel Wang,
Galaxy Mergers: major/minor wet/dry Hans-Walter Rix MPIA, Heidelberg … which galaxies are most shaped by mergers? … when do mergers matter for the SFR?
The Thick Disks of Spiral Galaxies as Relics from Gas-Rich, Turbulent, Clumpy Disks at High Redshifts Frédéric Bournaud, Bruce G. Elmegreen, and Marie.
KASI Galaxy Evolution Journal Club Comparing the Relation between Star Formation and Galaxy Mass in Different Environments - B. Vulcani et al. 2010, ApJ,
Cracking the mystery of galaxy and black hole formation: rachel somerville MPIA/STScI a Theorists’ Wish List for the next generation of Space Telescopes.
Galactic Stellar Population Structure and kinematics Alessandro Spagna Osservatorio Astronomico di Torino 26 Febbraio 2002.
Weidong Li Jesse Leaman Alex Filippenko Department of Astronomy University of California, Berkeley Nearby Supernova Rates from the Lick Observatory Supernova.
Next Topic, Brute Force Let’s go measure a lot of redshifts, assume z tells us the distance, and see what we can see. => The “z machine of Huchra and Geller.
Galactic Stellar Population Structure and kinematics
Black Hole Growth in the Local Universe
Mysteries of the Universe Fadeeva Tanya Kobegina Vika The 8 th Class School №196.
KASI Galaxy Evolution Journal Club